Friday, June 15, 2018

Photo of the Day: Make This Lakers Super Team Happen!

Paul George, Kawhi Leonard AND LeBron James playing on the Los Angeles Lakers?? Make it happen!!

A few hours ago, I found out that 2-time NBA All-Star Kawhi Leonard wants to be traded from the San Antonio Spurs...the team he's been with for about seven seasons (and won an NBA championship with in 2014). Leonard, a Los Angeles native, prefers to play for a team in his home town—which either means going to the Lakers or the Clippers, preferably the Lakers. Combine this report with the other one about LeBron James thinking about joining the Lake Show after leading the Cleveland Cavaliers back to the NBA Finals two weeks ago (only to fall to the Golden State Warriors for the third time in four years, one week ago today), and you have a doozy. Combine these reports with the one about Paul George wanting to leave the Oklahoma City Thunder to play in the City of Angels as well, and you have a major doozy.

LeBron James, Paul George and Kawhi Leonard all playing on the Lakers?! Make it happen! Don't toy with my emotions like that, basketball gods (and Jeanie Buss)! Carry on.

Thursday, June 14, 2018

Hayabusa2 Update: Asteroid Ryugu Begins to Reveal Itself...

An image of asteroid Ryugu that was taken from a distance of 920 kilometers...by JAXA's Hayabusa 2 spacecraft on June 13, 2018 (Japan Time).
JAXA

Ryugu Seen From a Distance of 920km (Press Release)

Hayabusa 2 is steadily approaching asteroid Ryugu. Figure 1 (above) shows a photograph of Ryugu taken on June 13, 2018 with the ONC-T (Optical Navigation Camera - Telescopic) from a distance of about 920km. The celestial body shining brightly in the center of the frame is Ryugu. The movement of Ryugu (in comparison to the background stars) can be seen by comparing this image with those taken on June 6 and June 10. The brightness of Ryugu is now about -6.6 mag (astronomical magnitude: a logarithmic scale for the apparent brightness for an object).

Figure 2 (below) shows the photograph taken with an exposure time of about 0.09 seconds. The part of the image that covers Ryugu is now about 10 pixels in diameter. We are describing the shape seen so far as a "dango"-type, as it looks like the round dango Japanese sweet dumpling made from rice flour (they taste delicious and we can recommend trying one). However, the shape does seem a little more angular.

These images were taken on June 13th, the same day that Hayabusa returned to Earth eight years ago. Just eight years later, Hayabusa 2 is less than 1000 km from asteroid Ryugu. We are looking forward to seeing what developments come next!

Source: Japan Aerospace Exploration Agency

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Another image of asteroid Ryugu that was taken from a distance of 920 kilometers...by JAXA's Hayabusa 2 spacecraft on June 13, 2018 (Japan Time).
JAXA

Wednesday, June 13, 2018

Photos of the Day: The MPR Raccoon...

A fan-made illustration that celebrates the MPR Raccoon's daring exploits atop the UBS Tower in St. Paul, Minnesota...on June 12 - 13, 2018.

Just thought I'd share these images, which were originally posted on Twitter, of the courageous raccoon that made her way to the top of the 25-story UBS Tower in St. Paul, Minnesota earlier today. The raccoon (nicknamed "MPR Raccoon" by Minnesota Public Radio news reporters who initially covered the animal's brave exploits), was stuck on the skyscraper for the past two days...having been scared off from a neighboring office block by city workers on Tuesday morning, only to start scaling the UBS building soon thereafter. I myself didn't notice the #MPRraccoon hashtag on Twitter till last night. Once I saw it, I kept refreshing the page till midnight as I waited for new tweets to appear reporting on the latest progress made by this furry daredevil.

A snapshot of MPR Raccoon scaling the side of the UBS Tower in St. Paul, Minnesota...on June 12, 2018.
Evan Frost | MPR News

I went to sleep around midnight after it became apparent that the raccoon was taking a nap on a ledge after she changed course and initially made her way a couple of stories down the UBS Tower. When I woke up around 7 this morning, I quickly retrieved my smartphone and clicked on the Twitter app...only to pleasantly see that MPR Raccoon was already on the rooftop of the skyscraper, and most likely sitting inside a cage feasting on cat food that was waiting for her!


Just like the feelings of other folks who also kept tabs on the trash panda's exploits, this happy conclusion was quite the morale booster! At a time when Donald Trump's latest destabilizing move is to legitimize a brutal communist dictator by meeting North Korean leader Kim Jong-un in Singapore (making history by showing an American president who's willing to make amends with an adversary that slaughtered millions of people in his own country, while at the same time shunning long-standing U.S. allies like Canada, France and Germany), it was refreshing to see a little creature beat the odds by accomplishing a daring feat that could've easily resulted in her death. MPR Raccoon exemplified that with determination, stamina and a little rest, anything is possible. Including getting through a lousy administration (and the complicit Republican Party that enables it) whose shenanigans have been wreaking havoc on America since the day Trump was sworn in. Happy Hump Day.

A snapshot of MPR Raccoon lying on a ledge at the Town Square Building in St. Paul, Minnesota...on June 12, 2018.
Evan Frost | MPR News

A snapshot of MPR Raccoon scaling the side of the UBS Tower in St. Paul, Minnesota...on June 12, 2018.
Ben - @Johnson88Ben on Twitter.com

A snapshot of MPR Raccoon sitting on a ledge at the UBS Tower in St. Paul, Minnesota...on June 12, 2018.
Paige Donnelly law - @donnelly_law on Twitter.com

A snapshot of MPR Raccoon about to reach the rooftop of the UBS Tower in St. Paul, Minnesota...on June 12, 2018.
D.P. - @@DPet_KARE11News on Twitter.com

A snapshot of MPR Raccoon sitting inside a cage after reaching the rooftop of the UBS Tower in St. Paul, Minnesota...on June 13, 2018.
Evan Frost | MPR News

MPR Raccoon scurries away after she is released from her cage following her rescue from the rooftop of the UBS Tower in St. Paul, Minnesota...on June 13, 2018.
Wildlife Management Services

Tuesday, June 12, 2018

F-35 Update: A Major Milestone Is Achieved for the Joint Strike Fighter...

The 300th F-35 Lightning II lifts off from the Lockheed Martin facility in Fort Worth Texas.
Lockheed Martin

Pentagon and Lockheed Martin Deliver 300th F-35 Aircraft (Press Release - June 11)

FORT WORTH, Texas, June 11, 2018 -- The F-35 Joint Program Office and Lockheed Martin delivered the 300th production F-35 aircraft, demonstrating the program's continued progress and momentum. The 300th aircraft is a U.S. Air Force F-35A, to be delivered to Hill Air Force Base, Utah.

"The F-35 weapons system is a key enabler of our National Defense Strategy and is providing our warfighters the combat proven, advanced capabilities they need to meet mission requirements," said Vice Admiral Mat Winter, program executive officer for the F-35 Joint Program Office. "The 300th production aircraft delivery is a significant milestone that highlights the effective F-35 Enterprise collaboration across the JPO, U.S. services, partners and industry. Moving forward, our F-35 team remains committed to driving costs down, quality up and faster delivery timelines across our development, production and sustainment lines of effort."

The first 300 F-35s include 197 F-35A conventional takeoff and landing (CTOL) variants, 75 F-35B short takeoff/vertical landing (STOVL) variants, and 28 F-35C carrier variants (CV) and have been delivered to U.S. and international customers. More than 620 pilots and 5,600 maintainers have been trained, and the F-35 fleet has surpassed more than 140,000 cumulative flight hours.

"This milestone is a testament to the hard work and dedication of our joint government and industry team as we collaborate to deliver transformational F-35 capabilities to the men and women in uniform," said Greg Ulmer, Lockheed Martin vice president and general manager of the F-35 program. "We are focused on reducing costs, increasing efficiencies, and ensuring the highest level of quality as we ramp to full rate production and sustainment of the operational fleet."

Increasing Production, Reducing Costs

As production volume increases and additional efficiencies are implemented, Lockheed Martin is on track to reduce the cost of an F-35A to $80 million by 2020, which is equal to or less than legacy 4th generation aircraft. With the incorporation of lessons learned, process efficiencies, production automation, facility and tooling upgrades, supply chain initiatives and more, the F-35 enterprise has already significantly reduced costs and improved efficiency. For example:

- The price of an F-35A has come down more than 60 percent from the first contract.

- Touch labor has been reduced by about 75 percent over the last five years.

- Production span time has decreased by about 20 percent since 2015.

The F-35 enterprise met its 2017 delivery target of 66 aircraft, representing more than a 40 percent increase from 2016. In 2018, the team is targeting 91 aircraft deliveries and is preparing to increase production volume year-over-year to hit a rate of approximately 160 aircraft in 2023.

Economic Impact

The F-35 is built by thousands of men and women in America and around the world. With more than 1,500 suppliers in 46 states and Puerto Rico, the F-35 program supports more than 194,000 direct and indirect jobs in the U.S. alone. The program also includes more than 100 international suppliers, creating or sustaining thousands of international jobs.

With stealth technology, supersonic speed, advanced sensors, weapons capacity and range, the F-35 is the most lethal, survivable and connected fighter aircraft ever built. More than a fighter jet, the F-35's ability to collect, analyze and share data is a powerful force multiplier that enhances all airborne, surface and ground-based assets in the battlespace and enables men and women in uniform to execute their mission and return home safe.

Source: Lockheed Martin

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Monday, June 11, 2018

Hayabusa2 Gets Closer To Its Asteroid Target...

An image of asteroid Ryugu that was taken from a distance of 1,500 kilometers...by JAXA's Hayabusa 2 spacecraft on June 10, 2018 (Japan Time).
JAXA

Ryugu Seen From a Distance of 1500km (Press Release)

Hayabusa 2 is continuing to approach asteroid Ryugu using optical navigation. Figure 1 (above) shows Ryugu photographed by the ONC-T (Optical Navigation Camera - Telescopic) on June 10, 2018, from a distance of about 1500km. The celestial body shining brightly in the center of the image is Ryugu. Compared with images taken on June 6, the position in the sky (relative to background stars) where Ryugu is visible has changed. The astronomical magnitude of Ryugu is now -5.7 mag.

Figure 2 (below) shows a photograph taken at approximately the same time but using an exposure of about 0.09 seconds. Here, only Ryugu is imaged as a point and the background stars are now too faint to be seen. In expanding the section of image that contains Ryugu, the asteroid can be seen to have a diameter of about 5 or 6 pixels but this is still not sufficient to see the shape. However, from this image is does seem that Ryugu is not elongated like Itokawa.

Hayabusa 2 will continue to draw closer to Ryugu. Please keep following us for future images!

Source: Japan Aerospace Exploration Agency

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Another image of asteroid Ryugu that was taken from a distance of 1,500 kilometers...by JAXA's Hayabusa 2 spacecraft on June 10, 2018 (Japan Time).
JAXA

Sunday, June 10, 2018

America's Oldest Active Mars Rover Braces Itself for Severe Weather on the Red Planet...

The blue dot in this image shows the location of NASA's Opportunity rover as a giant dust storm (photographed by the Mars Reconnaissance Orbiter) swirls across the surface of the Red Planet...on June 6, 2018.
NASA / JPL - Caltech / MSSS

Opportunity Hunkers Down During Dust Storm (News Release - June 9)

Science operations for NASA's Opportunity rover have been temporarily suspended as it waits out a growing dust storm on Mars.

NASA's Mars Reconnaissance Orbiter first detected the storm on Friday, June 1. As soon as the orbiter team saw how close the storm was to Opportunity, they notified the rover's team to begin preparing contingency plans.

In a matter of days, the storm had ballooned. It now spans more than 7 million square miles (18 million square kilometers) -- an area greater than North America -- and includes Opportunity's current location at Perseverance Valley. More importantly, the swirling dust has raised the atmospheric opacity, or "tau," in the valley in the past few days. This is comparable to an extremely smoggy day that blots out sunlight. The rover uses solar panels to provide power and to recharge its batteries.

Opportunity's power levels had dropped significantly by Wednesday, June 6, requiring the rover to shift to minimal operations.

This isn't Opportunity's first time hunkering down in bad weather: in 2007, a much larger storm covered the planet. That led to two weeks of minimal operations, including several days with no contact from the rover to save power. The project's management prepared for the possibility that Opportunity couldn't balance low levels of power with its energy-intensive survival heaters, which protect its batteries from Mars' extreme cold. It's not unlike running a car in the winter so that the cold doesn't sap its battery charge. There is a risk to the rover if the storm persists for too long and Opportunity gets too cold while waiting for the skies to clear.

Ultimately, the storm subsided and Opportunity prevailed. The Martian cold is believed to have resulted in the loss of Spirit, Opportunity's twin in the Mars Exploration Rover mission, back in 2010. Despite this, both rovers have vastly exceeded expectations: they were only designed to last 90 days each. Opportunity is in its 15th year; the team has operated the rover for more than 50 times longer than originally planned. Full dust storms like this one are not surprising, but are infrequent. They can crop up suddenly but last weeks, even months. During southern summer, sunlight warms dust particles, lifting them higher into the atmosphere and creating more wind. That wind kicks up yet more dust, creating a feedback loop that NASA scientists still seek to understand.

Mars Reconnaissance Orbiter and two other NASA spacecraft orbiting the Red Planet -- Odyssey and MAVEN -- routinely support rovers on the ground.

Source: Jet Propulsion Laboratory

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Full-size models of the Mars Exploration Rover and Sojourner rover (near the right side of this photo) at JPL...on May 20, 2017.

Saturday, June 09, 2018

2 of the 3 Closest Stars Outside Our Solar System May Not Be that Hostile to Any Habitable World Orbiting Them, After All...

Visible and X-ray photos of Alpha Centauri in a vast starfield...with the X-ray image taken by NASA's Chandra X-ray Observatory.
Optical: Zdenek Bardon; X-ray: NASA / CXC / Univ. of Colorado / T. Ayres et al.

Alpha Centauri: A Triple Star System about 4 Light Years from Earth (News Release - June 6)

A new study involving long-term monitoring of Alpha Centauri by NASA’s Chandra X-ray Observatory indicates that any planets orbiting the two brightest stars are likely not being pummeled by large amounts of X-ray radiation from their host stars. This is important for the viability of life in the nearest star system outside the Solar System. Chandra data from May 2nd, 2017 are seen in the pull-out, which is shown in context of a visible-light image taken from the ground of the Alpha Centauri system and its surroundings.

Alpha Centauri is a triple star system located just over four light years, or about 25 trillion miles, from Earth. While this is a large distance in terrestrial terms, it is three times closer than the next nearest Sun-like star.

The stars in the Alpha Centauri system include a pair called “A” and “B,” (AB for short) which orbit relatively close to each other. Alpha Cen A is a near twin of our Sun in almost every way, including age, while Alpha Cen B is somewhat smaller and dimmer but still quite similar to the Sun. The third member, Alpha Cen C (also known as Proxima), is a much smaller red dwarf star that travels around the AB pair in a much larger orbit that takes it more than 10 thousand times farther from the AB pair than the Earth-Sun distance. Proxima currently holds the title of the nearest star to Earth, although AB is a very close second.

The Chandra data reveal that the prospects for life in terms of current X-ray bombardment are actually better around Alpha Cen A than for the Sun, and Alpha Cen B fares only slightly worse. Proxima, on the other hand, is a type of active red dwarf star known to frequently send out dangerous flares of X-ray radiation, and is likely hostile to life. Planets in the habitable zone around Proxima receive an average dose of X-rays about 500 times larger than the Earth, and 50,000 times larger during a big flare.

Tom Ayres of the University of Colorado at Boulder presented these results at the 232rd meeting of the American Astronomical Society meeting in Denver, Colorado, and some of these results were published in January 2018 in the Research Notes of the American Astronomical Society. NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.

Source: NASA.Gov

Friday, June 08, 2018

Hayabusa2 Closes In On Its Asteroid Target...

An image of asteroid Ryugu that was taken from a distance of 2,600 kilometers...by JAXA's Hayabusa 2 spacecraft on June 6, 2018 (Japan Time).
JAXA

Ryugu Seen From a Distance of 2600km (Press Release - June 7)

On June 3, 2018, ion engine operation was completed and the final approach to the asteroid begun. By photographing the asteroid with the Optical Navigation Camera, optical navigation (precisely “hybrid navigation using optical and radiometric observations”) can be used to approach Ryugu while accurately estimating the trajectory of the spacecraft and asteroid.

Figure 1 above shows an image taken with the ONC-T (Optical Navigation Camera - Telescopic). This photo was taken on June 6 at approximately 04:15 JST from the spacecraft in the direction of Ryugu. Ryugu appears extremely bright due to a long exposure time of 178 seconds, which was used in order to image background stars. Because of this, Ryugu has become blurred and smears are generated. The brightness of Ryugu here is about -5 magnitude (a brightness scale used for stars).

In order to image Ryugu properly, a shorter exposure time is needed. Figure 2 (below) shows a photograph taken at approximately the same time with an exposure time of about 0.09 seconds. On Ryugu is seen as a point, without any stars in the background. An enlargement of that part of the image is seen on the left side of Figure 2, with the image of Ryugu being about 3 pixels in diameter.

The distance from the spacecraft to Ryugu at the time the images were taken is about 2600km. In the ONC-T image, one pixel is about 22 arcseconds. Therefore, in Figure 2, the length of one pixel would be approximately 0.3km. This means we still cannot yet know the shape of the asteroid.

Source: Japan Aerospace Exploration Agency

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Another image of asteroid Ryugu that was taken from a distance of 2,600 kilometers...by JAXA's Hayabusa 2 spacecraft on June 6, 2018 (Japan Time).
JAXA

Thursday, June 07, 2018

Curiosity Update: The Search for Life on Mars Has Made a Huge Breakthrough...

A self-portrait of NASA's Curiosity Mars rover, taken with a camera on her robotic arm on August 5, 2015.
NASA / JPL - Caltech / MSSS

NASA Finds Ancient Organic Material, Mysterious Methane on Mars (Press Release)

NASA’s Curiosity rover has found new evidence preserved in rocks on Mars that suggests the planet could have supported ancient life, as well as new evidence in the Martian atmosphere that relates to the search for current life on the Red Planet. While not necessarily evidence of life itself, these findings are a good sign for future missions exploring the planet’s surface and subsurface.

The new findings – “tough” organic molecules in three-billion-year-old sedimentary rocks near the surface, as well as seasonal variations in the levels of methane in the atmosphere – appear in the June 8 edition of the journal Science.

Organic molecules contain carbon and hydrogen, and also may include oxygen, nitrogen and other elements. While commonly associated with life, organic molecules also can be created by non-biological processes and are not necessarily indicators of life.

“With these new findings, Mars is telling us to stay the course and keep searching for evidence of life,” said Thomas Zurbuchen, associate administrator for the Science Mission Directorate at NASA Headquarters, in Washington. “I’m confident that our ongoing and planned missions will unlock even more breathtaking discoveries on the Red Planet.”

“Curiosity has not determined the source of the organic molecules,” said Jen Eigenbrode of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, who is lead author of one of the two new Science papers. “Whether it holds a record of ancient life, was food for life, or has existed in the absence of life, organic matter in Martian materials holds chemical clues to planetary conditions and processes.”

Although the surface of Mars is inhospitable today, there is clear evidence that in the distant past, the Martian climate allowed liquid water – an essential ingredient for life as we know it – to pool at the surface. Data from Curiosity reveal that billions of years ago, a water lake inside Gale Crater held all the ingredients necessary for life, including chemical building blocks and energy sources.

“The Martian surface is exposed to radiation from space. Both radiation and harsh chemicals break down organic matter,” said Eigenbrode. “Finding ancient organic molecules in the top five centimeters of rock that was deposited when Mars may have been habitable, bodes well for us to learn the story of organic molecules on Mars with future missions that will drill deeper.”

Seasonal Methane Releases

In the second paper, scientists describe the discovery of seasonal variations in methane in the Martian atmosphere over the course of nearly three Mars years, which is almost six Earth years. This variation was detected by Curiosity’s Sample Analysis at Mars (SAM) instrument suite.

Water-rock chemistry might have generated the methane, but scientists cannot rule out the possibility of biological origins. Methane previously had been detected in Mars' atmosphere in large, unpredictable plumes. This new result shows that low levels of methane within Gale Crater repeatedly peak in warm, summer months and drop in the winter every year.

"This is the first time we've seen something repeatable in the methane story, so it offers us a handle in understanding it," said Chris Webster of NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California, lead author of the second paper. "This is all possible because of Curiosity's longevity. The long duration has allowed us to see the patterns in this seasonal 'breathing.'"

Finding Organic Molecules

To identify organic material in the Martian soil, Curiosity drilled into sedimentary rocks known as mudstone from four areas in Gale Crater. This mudstone gradually formed billions of years ago from silt that accumulated at the bottom of the ancient lake. The rock samples were analyzed by SAM, which uses an oven to heat the samples (in excess of 900 degrees Fahrenheit, or 500 degrees Celsius) to release organic molecules from the powdered rock.

SAM measured small organic molecules that came off the mudstone sample – fragments of larger organic molecules that don’t vaporize easily. Some of these fragments contain sulfur, which could have helped preserve them in the same way sulfur is used to make car tires more durable, according to Eigenbrode.

The results also indicate organic carbon concentrations on the order of 10 parts per million or more. This is close to the amount observed in Martian meteorites and about 100 times greater than prior detections of organic carbon on Mars’ surface. Some of the molecules identified include thiophenes, benzene, toluene, and small carbon chains, such as propane or butene.

In 2013, SAM detected some organic molecules containing chlorine in rocks at the deepest point in the crater. This new discovery builds on the inventory of molecules detected in the ancient lake sediments on Mars and helps explains why they were preserved.

Finding methane in the atmosphere and ancient carbon preserved on the surface gives scientists confidence that NASA's Mars 2020 rover and ESA’s (European Space Agency's) ExoMars rover will find even more organics, both on the surface and in the shallow subsurface.

These results also inform scientists’ decisions as they work to find answers to questions concerning the possibility of life on Mars.

“Are there signs of life on Mars?” said Michael Meyer, lead scientist for NASA's Mars Exploration Program, at NASA Headquarters. “We don’t know, but these results tell us we are on the right track.”

This work was funded by NASA's Mars Exploration Program for the agency’s Science Mission Directorate (SMD) in Washington. Goddard provided the SAM instrument. JPL built the rover and manages the project for SMD.

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An image showing the drill site where NASA's Curiosity Mars rover found organic matter at Gale Crater, Curiosity's landing site.
NASA / JPL - Caltech / MSSS

Wednesday, June 06, 2018

Photos of the Day: Parker Gets Its Wings...

A snapshot of NASA's Parker Solar Probe after its twin solar arrays were installed on May 31, 2018...at Astrotech Space Operations in Titusville, Florida.
NASA / Johns Hopkins APL / Ed Whitman

Power Up: Solar Arrays Installed on NASA’s Mission to Touch the Sun (News Release)

NASA’s Parker Solar Probe depends on the Sun, not just as an object of scientific investigation, but also for the power that drives its instruments and systems. On Thursday, May 31, 2018, the spacecraft’s solar arrays were installed and tested. These arrays will power all of the spacecraft’s systems, including the suites of scientific instruments studying the solar wind and the Sun’s corona as well as the Solar Array Cooling System (SACS) that will protect the arrays from the extreme heat at the Sun.

“Unlike solar-powered missions that operate far from the Sun and are focused only on generating power from it, we need to manage the power generated along with the substantial heat that comes from being so close to the Sun,” said Andy Driesman, project manager from the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland. “When we’re out around the orbit of Venus, we fully extend the arrays to get the power we need. But when we’re near the Sun, we tuck the arrays back until only a small wing is exposed, and that portion is enough to provide needed electrical power.”

The solar arrays are cooled by a gallon of water that circulates through tubes in the arrays and into large radiators at the top of the spacecraft. They are just over three and a half feet (1.12 meters) long and nearly two and a half feet (0.69 meters) wide. Mounted on motorized arms, the arrays will retract almost all of their surface behind the Thermal Protection System – the heat shield – when the spacecraft is close to the Sun. The solar array installation marks some of the final preparation and testing of Parker Solar Probe leading up to the mission’s July 31 launch date.

Source: Johns Hopkins Applied Physics Laboratory

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Parker Solar Probe team engineers inspect one of the twin solar arrays installed aboard the spacecraft on May 31, 2018...at Astrotech Space Operations in Titusville, Florida.
NASA / Johns Hopkins APL / Ed Whitman

Parker Solar Probe team engineers use a laser to illuminate the cells on the twin solar arrays installed aboard the spacecraft on May 31, 2018...at Astrotech Space Operations in Titusville, Florida.
NASA / Johns Hopkins APL / Ed Whitman

Parker Solar Probe team engineers use a laser to illuminate the cells on the twin solar arrays installed aboard the spacecraft on May 31, 2018...at Astrotech Space Operations in Titusville, Florida.
NASA / Johns Hopkins APL / Ed Whitman